Star · F9V
TOI-3474
TOI-3474 is a main-sequence star of spectral type F9V in the constellation Lupus, 1,370 light-years from the Sun. It is orbited by 1 confirmed exoplanet(s).
| Constellation | Lupus |
|---|---|
| Distance | 1,370 light-years (420.1 pc) |
| Apparent magnitude | magnitude 12.53 |
| Absolute magnitude | magnitude 4.41 |
| Spectral type | F9V |
| Surface temperature | 6,020 K |
| Luminosity | 1.86 L☉ |
| Radius | 1.26 R☉ |
| Mass | 1.12 M☉ |
| Age | 4.7 billion years |
| Metallicity [Fe/H] | 0.15 |
| Right ascension (J2000) | 15h 34m 00.8s |
| Declination (J2000) | −47° 57′ 49″ |
| Space velocity (relative to the Sun) | 17.6 km/s |
In the sky
A telescope is needed to see it: its apparent magnitude is 12.53. Visible from the whole Southern Hemisphere and north to latitude 42° N. South of latitude 42° S it never sets. It stands highest at midnight in May, the best time to observe it.
Through a telescope from Earth
Light's journey
The light you see tonight set out around the year 656. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 24 million years.
The Sun seen from there
From a planet around TOI-3474, the Sun would look like a star of magnitude 12.95, in the direction where our sky has the constellation Perseus. It would be invisible to the naked eye.
Planets
- TOI-3474 b 3.88-day orbit · 14.7 R⊕
Stellar parameters from the NASA Exoplanet Archive; position and brightness from the HYG / AT-HYG catalogue.